### Methane on Mars
Scientists have detected trace amounts of methane () in the Martian atmosphere. Because methane is rapidly destroyed by ultraviolet (UV) radiation, its presence indicates an active source. Two hypotheses explain the origin and behavior of Martian methane.
Hypothesis 1
Methane is produced biologically by subsurface methanogenic microbes. These microbes reside in deep, liquid-water aquifers insulated by a thick cryosphere. The liquid water is maintained at temperatures around to by modest geothermal heat. The microbes combine carbon dioxide () and hydrogen () to produce energy and release as a metabolic waste product. The observed seasonal fluctuations in atmospheric methane concentration are due to variations in microbial metabolic rates, which increase during the warmer Martian summer.
Hypothesis 2
Methane is produced abiotically through serpentinization, a geochemical reaction. Deep within the crust, water heated to temperatures between and reacts with olivine-rich volcanic rocks to produce , which then reacts with dissolved carbon oxides to form . This methane becomes trapped in clathrate hydrates (crystalline water-ice cages) within the cryosphere. The observed seasonal fluctuations are not due to active production, but rather the thermal destabilization of these shallow clathrate hydrates, which release trapped methane into the atmosphere as the ground warms during summer.
Match each parameter of Martian methane production and behavior on the left with the specific point of disagreement between Hypothesis 1 and Hypothesis 2 on the right.
- The primary origin of the methane sourceHypothesis 1 proposes a biological metabolic origin, whereas Hypothesis 2 proposes an abiotic geochemical reaction between crustal rocks and water.
- The temperature conditions required for methane generationHypothesis 1 requires moderate temperatures suitable for microbial life ( to ), whereas Hypothesis 2 requires high temperatures ( to ) to drive serpentinization.
- The cause of seasonal fluctuations in atmospheric methane levelsHypothesis 1 attributes variations to changes in active microbial production rates, whereas Hypothesis 2 attributes them to the physical release of trapped gas from destabilized clathrate hydrates.